LMC N49
{{Short description|Supernova remnant in the constellation Dorado}}
{{sky|05|26|01.00|-|66|05|06.0|165000}}
{{Infobox nebula
|name = LMC N49
|image = Sig06-030.jpg
|caption =
|credit =
|type = Supernova remnant
|type2 =
|epoch = J2000.0
|subtype =
|class =
|dist_pc =
|dist_z =
|appdia =
|size_v =
|constellation = Dorado
|radius_ly =
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|notes =
|names = LMC N49, PKS 0525-66, PKS B0525-661, PKS J0525-6604, SNR J052559-660453
}}
{{commonscat|N49}}
N49 or LMC N49 (PKS 0525-66, PKS B0525-661, PKS J0525-6604, SNR J052559-660453), also known as Brasil Nebula,Sky & Telescope, August 2004, page 12 is the brightest supernova remnant in the Large Magellanic Cloud, approximately 160,000 light-years from Earth. Its form has been assessed to be roughly 5,000 years old.
The latest pictures of N49 by the Chandra X-ray Observatory have revealed a bullet-shaped object traveling at about 5 million miles an hour away from a bright X-ray and gamma-ray point source, probably a neutron star with an extremely powerful magnetic field, known as a soft gamma repeater. A particularly strong gamma-ray burst from LMC N49 was detected on March 5, 1979.
References
{{reflist|refs=
{{cite simbad |title= SNR J052559-660453 }}
{{cite web |url= http://chandra.harvard.edu/photo/2010/n49/ |title=N49: Stellar Shrapnel Seen in Aftermath of Explosion |author=Chandra X-ray Observatory |date=2010-05-24 |accessdate=2015-10-15}}
}}
- Harvard-Smithsonian Center for Astrophysics, [https://www.cfa.harvard.edu/ssp/extreme_astrophysics/n49.html "N49: A supernova remnant in the Large Magellanic Cloud"]
{{Dorado}}
{{DEFAULTSORT:LMC N49}}